- Introduction
- emission processes
- line emissivities/intensities using PyNeb
- energy balance in HII regions
- atomic data
- deredenning
- physical properties of HII regions
- plasma diagnostics
- abundances by direct method (ionic abundances, ICFs)
- strong line methods, calibrations (empirical, theoretical)
- Cloudy and pyCloudy
- simple model, grid of models. Comparing making N models and using grid from Cloudy.
- model fitting observations and limits
- grids of models (2)
- Strong lines methods and BOND models (Natalia Vale-Asarie)
- 3MdB and 3MdBs
- combined models
- Topologically equivalent models
- 3D models, ionization structure.